SDO HMI 2014-09-22 16:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.43 | 25.67 | 5.51 | 19.66 | -15.03 | 249.85 | -44.87 | 116.67 | 0.7639 | 157.6 | 70.1 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.72 | -15.64 | 251.88 | -42.84 | 118.40 | 0.7466 | 335.0 | 311.7 | |
| 5.93 | 15.84 | 4.39 | 11.75 | -15.23 | 251.78 | -42.94 | 117.84 | 0.7457 | 863.8 | 509.5 | |
| 1.50 | -2.00 | 1.12 | -2.00 | -15.40 | 251.60 | -43.12 | 117.96 | 0.7484 | 450.2 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.59 | -13.65 | 251.39 | -43.33 | 115.70 | 0.7423 | 574.0 | 462.3 | |
| 0.00 | 0.97 | 0.00 | 0.78 | -15.69 | 247.70 | -47.02 | 116.35 | 0.7882 | -482.0 | -346.5 | |
| 0.00 | 0.80 | 0.00 | 0.64 | -14.20 | 246.75 | -47.97 | 114.16 | 0.7914 | -537.0 | -478.0 | |
| 0.00 | 2.39 | 0.00 | 1.92 | -13.98 | 246.77 | -47.95 | 113.90 | 0.7904 | -610.0 | -544.3 | |
| 0.00 | 0.71 | 0.00 | 0.59 | -15.29 | 245.81 | -48.91 | 115.02 | 0.8045 | -531.0 | -413.9 | |
| 0.00 | 1.59 | 0.00 | 1.32 | -14.59 | 245.75 | -48.97 | 114.18 | 0.8025 | -627.0 | -522.7 | |
| 0.00 | 0.80 | 0.00 | 0.67 | -15.23 | 245.01 | -49.71 | 114.62 | 0.8117 | -356.0 | -372.8 | |
| 0.00 | 0.80 | 0.00 | 0.68 | -14.84 | 244.06 | -50.66 | 113.78 | 0.8191 | 225.0 | 177.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |